173 citations · 978 across the 33 of their papers we have counts for
33 papers
Magnetohydrodynamic/Kinetic Modeling of the Interaction between the Solar Wind and the Local Interstellar Medium with He, He, and Pickup H ions and H, He Atoms
Federico Fraternale, Nikolai V. Pogorelov, Ratan K. Bera
The interaction of the solar wind with the local interstellar medium (LISM) spans a wide range of interacting particle populations, energies, and scales. Sophisticated models are r…
Rotation of a Stealth CME on 2012 October 5 Observed in the Inner Heliosphere
Sandeep Kumar, Dinesha V. Hegde, Nandita Srivastava +3
Coronal Mass Ejections (CMEs) are subject to changes in their direction of propagation, tilt, and other properties. This is because CMEs interact with the ambient solar wind and ot…
Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R
Samuel T. Badman, Pete Riley, Shaela I. Jones +11
Drawing connections between heliospheric spacecraft and solar wind sources is a vital step in understanding the evolution of the solar corona into the solar wind and contextualizin…
Improving the Arrival Time Estimates of Coronal Mass Ejections by Using Magnetohydrodynamic Ensemble Modeling, Heliospheric Imager data, and Machine Learning
Talwinder Singh, Bernard Benson, Syed A. Z. Raza +4
The arrival time prediction of Coronal mass ejections (CMEs) is an area of active research. Many methods with varying levels of complexity have been developed to predict CME arriva…
A data-driven physics-based transport model of solar energetic particles accelerated by coronal mass ejection shocks propagating through the solar coronal and heliospheric magnetic fields
Ming Zhang, Lei Cheng, Ju Zhang +5
In an effort to develop computational tools for predicting radiation hazards from solar energetic particles (SEPs), we have created a data-driven physics-based particle transport m…
Using TeV Cosmic Rays to probe the Heliosphere's Boundary with the Local Interstellar Medium
Paolo Desiati, Juan Carlos Díaz Vélez, Gwenael Giacinti +4
The heliosphere is the magnetic structure formed by the Sun's atmosphere extending into the local interstellar medium (ISM). The boundary separating the heliosphere from the ISM is…